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Symplectic integration algorithms have become popular in recent years in long-term orbital integrations because these algorithms enforce certain conservation laws that are intrinsic to Hamiltonian systems. For problems with large variations…

天体物理学 · 物理学 2007-05-23 Man Hoi Lee , Martin J. Duncan , Harold F. Levison

We present a new mixed variable symplectic (MVS) integrator for planetary systems, that fully resolve close encounters. The method is based on a time regularisation that allows keeping the stability properties of the symplectic integrators,…

地球与行星天体物理 · 物理学 2019-07-31 Antoine C. Petit , Jacques Laskar , Gwenaël Boué , Mickaël Gastineau

In recent decades, there have been many attempts to construct symplectic integrators with variable time steps, with rather disappointing results. In this paper we identify the causes for this lack of performance, and find that they fall…

计算物理 · 物理学 2015-05-30 A S Richardson , J M Finn

Symplectic N-body integrators are widely used to study problems in celestial mechanics. The most popular algorithms are of 2nd and 4th order, requiring 2 and 6 substeps per timestep, respectively. The number of substeps increases rapidly…

天体物理学 · 物理学 2009-10-31 J. E. Chambers , M. A. Murison

Symplectic integration algorithms are well-suited for long-term integrations of Hamiltonian systems because they preserve the geometric structure of the Hamiltonian flow. However, this desirable property is generally lost when adaptive…

天体物理学 · 物理学 2025-10-20 Miguel Preto , Scott Tremaine

In this work we propose a new numerical approach to distinguish between regular and chaotic orbits in Hamiltonian systems, based on the simultaneous integration of both the orbit and the deviation vectors using a symplectic scheme, hereby…

混沌动力学 · 物理学 2015-03-17 Anne-Sophie Libert , Charles Hubaux , Timoteo Carletti

We show that when time-reversible symplectic algorithms are used to solve periodic motions, the energy error after one period is generally two orders higher than that of the algorithm. By use of correctable algorithms, we show that the…

数学物理 · 物理学 2009-11-10 S. R. Scuro , S. A. Chin

The usual explicit finite-difference method of solving partial differential equations is limited in stability because it approximates the exact amplification factor by power-series. By adapting the same exponential-splitting method of…

数值分析 · 数学 2012-06-11 Siu A. Chin

We suggest a numerical integration procedure for solving the equations of motion of certain classical spin systems which preserves the underlying symplectic structure of the phase space. Such symplectic integrators have been successfully…

统计力学 · 物理学 2007-05-23 Robin Steinigeweg , Heinz-Jürgen Schmidt

It has previously been shown that varying the numerical timestep during a symplectic orbital integration leads to a random walk in energy and angular momentum, destroying the phase space-conserving property of symplectic integrators. Here…

天体物理仪器与方法 · 物理学 2015-05-20 Nathan A. Kaib , Thomas Quinn , Ramon Brasser

Many force-gradient explicit symplectic integration algorithms have been designed for the Hamiltonian $H=T (\mathbf{p})+V(\mathbf{q})$ with kinetic energy $T(\mathbf{p})=\mathbf{p}^2/2$ in the existing references. When the force-gradient…

数值分析 · 数学 2021-11-10 Lina Zhang , Xin Wu , Enwei Liang

Dependable numerical results from long-time simulations require stable numerical integration schemes. For Hamiltonian systems, this is achieved with symplectic integrators, which conserve the symplectic condition and exactly solve for the…

等离子体物理 · 物理学 2015-06-17 Stephen D. Webb

Reliable studies of the long-term dynamics of planetary systems require numerical integrators that are accurate and fast. The challenge is often formidable because the chaotic nature of many systems requires relative numerical error bounds…

地球与行星天体物理 · 物理学 2023-06-07 Richard E. Zeebe

Symplectic integrators are widely used for the study of planetary dynamics and other $N$-body problems. In a study of the outer Solar system, we demonstrate that individual symplectic integrations can yield biased errors in the semi-major…

地球与行星天体物理 · 物理学 2021-04-15 David M. Hernandez , Eric Agol , Matthew J. Holman , Sam Hadden

We implement and investigate the numerical properties of a new family of integrators connecting both variants of the symplectic Euler schemes, and including an alternative to the classical symplectic mid-point scheme, with some additional…

数值分析 · 数学 2015-08-14 Hugo Jiménez-Pérez , Jean-Pierre Vilotte , Barbara Romanowicz

Calculating the long term solution of ordinary differential equations, such as those of the $N$-body problem, is central to understanding a wide range of dynamics in astrophysics, from galaxy formation to planetary chaos. Because generally…

天体物理仪器与方法 · 物理学 2018-01-23 David M. Hernandez , Edmund Bertschinger

Most numerical integration algorithms are not designed specifically for Hamiltonian systems and do not respect their characteristic properties, which include the preservation of phase space volume with time. This can lead to spurious…

天体物理学 · 物理学 2015-06-24 David JD Earn

Symplectic integrators evolve dynamical systems according to modified Hamiltonians whose error terms are also well-defined Hamiltonians. The error of the algorithm is the sum of each error Hamiltonian's perturbation on the exact solution.…

数学物理 · 物理学 2008-11-26 Siu A. Chin

Symplectic integration methods based on operator splitting are well established in many branches of science. For Hamiltonian systems which split in more than two parts, symplectic methods of higher order have been studied in detail only for…

We introduce a class of fourth order symplectic algorithms that are ideal for doing long time integration of gravitational few-body problems. These algorithms have only positive time steps, but require computing the force gradient in…

天体物理学 · 物理学 2007-05-23 Siu A. Chin , C. R. Chen
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